skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: THE INTRINSIC FRACTIONS AND RADIO PROPERTIES OF LOW-IONIZATION BROAD ABSORPTION LINE QUASARS

Journal Article · · Astrophysical Journal
 [1];  [2]
  1. Homer L. Dodge Department of Physics and Astronomy, University of Oklahoma, Norman, OK 73019 (United States)
  2. GEPI, Observatoire de Paris, CNRS, University of Paris Diderot, 5 Place Jules Janssen, F-92195 Meudon (France)

Low-ionization (Mg II, Fe II, and Fe III) broad absorption line quasars (LoBALs) probe a relatively obscured quasar population and could be at an early evolutionary stage for quasars. We study the intrinsic fractions of LoBALs using the Sloan Digital Sky Survey (SDSS), Two Micron All Sky Survey, and Faint Images of the Radio Sky at Twenty cm survey. We find that the LoBAL fractions of the near-infrared (NIR) and radio samples are approximately 5-7 times higher than those measured in the optical sample. This suggests that the fractions measured in the NIR and radio bands are closer to the intrinsic fractions of the populations, and that the optical fractions are significantly biased due to obscuration effects, similar to high-ionization broad absorption line quasars (HiBALs). Considering a population of obscured quasars that do not enter the SDSS, which could have a much higher LoBAL fraction, we expect that the intrinsic fraction of LoBALs could be even higher. We also find that the LoBAL fractions decrease with increasing radio luminosities, again, similarly to HiBALs. In addition, we find evidence for increasing fractions of LoBALs toward higher NIR luminosities, especially for FeLoBALs with a fraction of {approx}18% at M{sub K{sub s}}< -31 mag. This population of NIR-luminous LoBALs may be at an early evolutionary stage of quasar evolution. To interpret the data, we use a luminosity-dependent model for LoBALs that yields significantly better fits than those from a pure geometric model.

OSTI ID:
22092141
Journal Information:
Astrophysical Journal, Vol. 757, Issue 2; Other Information: Country of input: International Atomic Energy Agency (IAEA); ISSN 0004-637X
Country of Publication:
United States
Language:
English

Similar Records

Fraction of broad absorption line quasars in different radio morphologies
Journal Article · Thu Jan 27 00:00:00 EST 2022 · Monthly Notices of the Royal Astronomical Society · OSTI ID:22092141

Near-IR Spectroscopy of Luminous LoBAL Quasars at 1 < z < 2.5
Journal Article · Fri Oct 20 00:00:00 EDT 2017 · Astrophysical Journal · OSTI ID:22092141

SDSS J1254+0846: A BINARY QUASAR CAUGHT IN THE ACT OF MERGING
Journal Article · Sat Feb 20 00:00:00 EST 2010 · Astrophysical Journal · OSTI ID:22092141